Proceedings of the 34th International Cosmic Ray Conference — PoS(ICRC2015) 2016
DOI: 10.22323/1.236.0255
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Depth of Maximum Development of Extensive Air Showers by Radio Emission Data at Yakutsk EAS Array

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(7 citation statements)
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“…• The features of the energy spectrum have been confirmed with improved statistics. The existence of the low energy ankle at ∼ 10 16 eV and of the second knee at ∼ 10 17 eV have been confirmed by IceCube [13], Yakutsk [11], KASKADE-Grande [10] and the TALE telescopes of TA [16]. The measurements of the position of the ankle at 5 × 10 18 eV by Auger [20,21] and TA [19,16] are in excellent agreement.…”
Section: Discussionmentioning
confidence: 71%
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“…• The features of the energy spectrum have been confirmed with improved statistics. The existence of the low energy ankle at ∼ 10 16 eV and of the second knee at ∼ 10 17 eV have been confirmed by IceCube [13], Yakutsk [11], KASKADE-Grande [10] and the TALE telescopes of TA [16]. The measurements of the position of the ankle at 5 × 10 18 eV by Auger [20,21] and TA [19,16] are in excellent agreement.…”
Section: Discussionmentioning
confidence: 71%
“…Unfortunately this quantity cannot be measured directly but has to be inferred from the measurement of the properties of the atmospheric showers, an inference affected by the large systematic uncertainties related to the hadronic interaction models. The mean value of logarithm of the mass number <ln A> at energies below 10 17 eV has been measured by the IceCube collaboration using coincident events in IceTop and the deep-ice detector [13], and with the Small Cherenkov Array in Yakutsk [24]. The measurements are shown in Figure 7 and both confirm that the composition becomes heavier from a few times 10 15 eV to 10 17 eV.…”
Section: The Mass Compositionmentioning
confidence: 81%
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